Results 131 to 140 of about 1,105,860 (262)

Source Region of the Solar Wind: Statistics of the Doppler Velocities at the Chromosphere

open access: yesThe Astrophysical Journal Letters
The solar wind has been extensively studied recently with in situ observations, and the understanding of its counterpart near the solar surface has also progressed significantly.
Fu Yu   +10 more
doaj   +1 more source

An In-depth Analysis of Quiet-Sun IRIS Brightenings

open access: yesThe Astrophysical Journal
Small-scale brightenings are ubiquitous, dynamic, and energetic phenomena found in the chromosphere. An advanced filter-detection algorithm applied to high-resolution observations from the Interface Region Imaging Spectrograph enables the detection of ...
Llŷr Dafydd Humphries   +2 more
doaj   +1 more source

IRIS2+: A Comprehensive Database of Stratified Thermodynamic Models in the Low Solar Atmosphere

open access: yesThe Astrophysical Journal Supplement Series
We present the most comprehensive collection of stratified-in-optical-depth thermodynamic models of the lower solar atmosphere. This database, named IRIS ^2+ , consists of 40,320 synthetic representative profiles (RPs) and their corresponding ...
Alberto Sainz Dalda   +3 more
doaj   +1 more source

Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]

open access: yesNat Commun
Cang T   +13 more
europepmc   +2 more sources

Variations in Dominant Wave Period in the Solar Atmosphere

open access: yesThe Astrophysical Journal
Waves are an integral part of the solar atmosphere, and their characteristics (e.g., dominant period, range of periods, power, and phase angle) change on a diverse spatiotemporal scale.
Pradeep Kayshap   +3 more
doaj   +1 more source

The Effect of Plasma-β on the Heating Mechanisms during Magnetic Reconnection in Partially Ionized Low Solar Atmosphere

open access: yesThe Astrophysical Journal
We performed numerical simulations of magnetic reconnection with different strengths of magnetic fields from the solar photosphere to the upper chromosphere.
Abdullah Zafar   +7 more
doaj   +1 more source

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